Ozone vertical distribution on Mars from SPICAN/MEX UV occultations
Abstract : We have achieved a four-year cli- matology of the O3 vertical distribution using SPICAM UV occultations. The climatology con- firms the overall behaviour of O3, but reveals some discrepancies in comparison with a global climate model.
We are presenting here a simple way to overcome the problem when comparing models and observations; direct comparison of slant profiles (i.e., without doing the vertical inversion).
Cited literature [7 references]
https://hal-insu.archives-ouvertes.fr/insu-02333762
Contributor : Catherine Cardon <>
Submitted on : Friday, October 25, 2019 - 3:31:18 PM
Last modification on : Friday, January 10, 2020 - 3:42:35 PM
Document(s) archivé(s) le : Sunday, January 26, 2020 - 4:39:50 PM
Contributor : Catherine Cardon <>
Submitted on : Friday, October 25, 2019 - 3:31:18 PM
Last modification on : Friday, January 10, 2020 - 3:42:35 PM
Document(s) archivé(s) le : Sunday, January 26, 2020 - 4:39:50 PM
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